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Dust: conservation of rho n tensor n is equivalent to continuity and inertial flow
Statement
Let be open, let be with , let be a field which is future timelike and satisfies everywhere (a future unit timelike field, Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(c)), and set (a symmetric field). Then, on , (a) if and only if both (continuity) and (inertial flow); (b) if is allowed to vanish, the implication is asserted only on the open set , and no assertion is made where ; (c) Under the conservation hypothesis in (a), if is an interval and is a curve with for all (an integral curve of ), then : the flow lines of an inertial unit field are affine straight lines in the affine structure of . For the nonnegative-density branch in (b), the same conclusion holds for an integral curve whose image lies in , under conservation there. The lemma is the exact mathematical content of the dust equations; it asserts no matter model, no interaction and no empirical fact. No choice principle is used.
Facts & Assumptions
Given: The affine Minkowski model with fixed inertial chart and coordinate partial derivatives (Oriented time-oriented affine Minkowski space (the spacetime primitives), Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space, Directional derivatives and partial derivatives of a map ), an open , fields and with ; and indices are raised and lowered with the constant (Norms of four-velocity and four-acceleration, and the observer rest-space decomposition,(c)). For a field the expression is the coordinate form of the flat covariant derivative (The flat covariant derivative on affine Minkowski space and fields along curves). For a symmetric type- field one writes and calls conserved when (C^k tensor fields on affine Minkowski space and their inertial components).
Product rule for coordinate partial derivatives of products of functions: . (Sums, scalar multiples, products and quotients: , , , and when , Directional derivatives and partial derivatives of a map )
If is an interval and is continuous on and differentiable at every interior point with there, then is constant on . (A function continuous on an interval whose derivative vanishes at every interior point of is constant on ; consequently two such functions with the same derivative differ by a constant)
Chain rule: a curve composed with a field is and its derivative is obtained by composing the derivative of the field with the curve derivative; concretely . (The chain rule for total derivatives: )
Proof
Algebraic identity. Since and are , [F1] gives with , the continuity expression.
Contraction identity. Because is constant, its derivative vanishes: , hence multiplying by and summing, ; likewise and .
Forward direction of (a) and clause (b). Assume on . Contracting the identity of step 1.1 with and using step 1.2 gives , hence . Substituting back gives for every . If everywhere, division by gives on ; if only is assumed, the same conclusion holds on the open set and no claim is made where .
Reverse direction of (a). Conversely, if and on , then step 1.1 gives on .
Clause (c). Let be a curve with . By [F3], , which vanishes under the conservation hypothesis by step 2.1 (or, in the nonnegative-density branch, at every with by step 2.1 applied there). Hence every component has zero derivative at every interior point of , and [F2] gives that is constant; applying [F2] to the function , whose derivative vanishes, gives for all and every . Thus is an affine straight line and on .
Steps 2.1 and 2.2 prove (a), step 2.1 proves the restricted implication (b), and step 3.1 proves (c) and its branch on . The argument is a pointwise component computation with the product rule and the constancy of ; it asserts no matter model, no interaction, no dynamics of beyond the displayed equations and no empirical fact, and it uses no choice principle.
Depends on
Norms of four-velocity and four-acceleration, and the observer rest-space decomposition
C^k tensor fields on affine Minkowski space and their inertial components
The flat covariant derivative on affine Minkowski space and fields along curves
Directional derivatives and partial derivatives of a map
Sums, scalar multiples, products and quotients: , , , and when
The chain rule for total derivatives:
Lorentz forms of inertia (3,1,0) on a 4-dimensional real vector space
Oriented time-oriented affine Minkowski space (the spacetime primitives)
A function continuous on an interval whose derivative vanishes at every interior point of is constant on ; consequently two such functions with the same derivative differ by a constant
Dependency tree · 2 levels
Sources
- B. Crowell, Special Relativity, revision 2020-12-10 (author-published undergraduate textbook, 246 PDF pages); signature (+---) converted to (-+++) and c = 1 formulas converted to x^0 = c t; Chapter 9 pp. 179-197: 9.1 pp. 179-182 (current vector, flux, charge conservation), 9.2 pp. 183-191 (stress-energy tensor, conservation and flux, symmetry, dust, rank-2 transformation law, pressure, perfect fluid, worked examples, energy conditions), 9.3 pp. 192-197 (Gauss's theorem, integral conservation laws, the energy-momentum vector, angular momentum); the printed 9.2.8 dominant energy condition p. 191 has the defective |P| > rho and is not used
- D. Tong, General Relativity, University of Cambridge Part III Mathematical Tripos (Michaelmas Term 2019); c = 1 formulas converted to x^0 = c t; 4.5.1-4.5.5 printed pp. 181-191: scalar-field action (4.42)-(4.43) and equation of motion, Hilbert energy-momentum tensor (4.46), diffeomorphism invariance and conservation (4.50), flat-space Noether form, scalar tensor (4.51), Maxwell tensor (4.52), perfect fluid (4.53) with conservation equations (4.54)-(4.55), and the flat-space conserved-charge box argument of 4.5.5
- S. M. Carroll, Lecture Notes on General Relativity, arXiv:gr-qc/9712019v1 (1997), Chapter 1 printed pp. 28-30 (energy-momentum tensor, dust T^{mu nu}=rho U^mu U^nu (1.106), perfect fluid (1.107)-(1.110), scalar and Maxwell tensors (1.111)-(1.112), conservation (1.113) with the remark that the proof follows from each matter model's equations of motion) and Chapter 5 printed pp. 138-139 (on-shell conservation from diffeomorphism invariance with compact-support variations, (5.34)-(5.38))